Open Access

This article has an erratum: [https://doi.org/10.1051/0004-6361/202037739e]


Fig. 4.

image

Red: for each facular index, the F-to-SA solar cycle amplitude ratio, relative to cycle 22, as a function of SA cycle amplitude. The dots represent the individual cycle values, determined using the model reconstruction of F from SA. The error bars and curves denote the corresponding 1σ uncertainty and quadratic polynomial fit. Grey: the F-to-S cycle amplitude ratio-versus-S cycle amplitude profiles for the SN1, SN2, SG1 and SG2. The various sunspot indices are rescaled to the SA scale to allow a direct comparison. Only the values from cycles 12 to 22, where the five sunspot index time series overlap, are depicted. The horizontal line marks the cycle 22 level (i.e. unity). See Sect. 4.2 for details.

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